362
Müller und Kempf, Photometrische Durchmusterung
362
R.D.
Sternzeit
I
II
III
1
IV
/
z
log sin 2 ,/
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
9°34 2 4
15h 22 m
31°°
29-4
31°°
2784
29870
5080
9.3900
9.4382
14 3180
15 25
23-4
23.O
26.4
22.0
23.70
42.0
9.2083
9.2364
0.0711
+ 0.18
6.61
13 3292
15 27
29.5
26.5
31-oj
27.O
28.50
42.7
9-3573
9.3868
0.0793
— 0.20
6.23
13 3295
15 29
29.7
27.4
32.8
27.6
29.38
42.7
9-38i5
9.41 IO
0.1035
— O.26
6.17
12 3161
15 31
26.0
20.0
20.0
I 7.O
20.75
44.1
9.0987
9-1312
0.1763
+ O.44
6.87
10 3153
15 33
19.0
16.4
17.6
16.O
17-25
46.1
8.9442
8.9815
0.3260
4- 0.81
7.24
10 3142
15 35
2 6.6
24.6
25.0
2 1.2
24-35
45-3
9-2305
9.2658
0.0417
4“ O.IO
6-53
9 3203
15 37
23.6
2O.9
24-5
l8.6
21.90
43-7
9-1434
9-1750
9 3424
15 40
31.0
29-5
30.9
25-4
29.20
48.2
9.3766
9-4195
Mittel aus den Vergleichsternbeobachtungen: 9.3205; 9.3048; 9.2972. Zur Reduction benutzt: 9.3075.
Zone 594. 1892 Jnni 7.
Beobachter: Müller.
Photometer:
Ci. Vergleichsterne: Nr. 33 und Nr. 35. Luft:
I.
7°3023
i6 h 6 m
3 2?0
2983
2884
3186
30832
4580
9.4063
9.4409
11 315 6
16 9
23.2
23-5
22.0
23-7
23.10
43-4
9 -i 873
9.2183
14 3049
16 11
27.8
28.7
28.0
26.6
27.78
38.1
9-3369
9-3582
0.0233
— 0.06
4-77
2 311 8
16 13
42.5
40.7
41.2
43-2
41.90
50.3
9-6493
9.6984
0-3635
— 0.91
3-92
5 3223
16 15
15.6
15-7
16.4
15-4
I5-78
46.7
8.8689
8.9077
0.4272
4-1.07
5-90
11 3008
16 17
24.9
24.8
24.4
25.0
24.78
40.7
9.2447
9.2704
0.0645
4- 0.16
4.99
8 3271
16 18
20.8
20.1
2I.7
24.6
21.80
43-8
9.1396
9-1715
0.1634
+ 0.41
5-24
5 3272
l6 20
21.5
20.7
2O.4
21.1
20.92
47.2
9-io55
9.1456
0.1893
+ 0.47
5-30
7 3023
l6 22
29-3
30.0
32-3
33-5
31.28
45-5
9-4307
9.4665
11 315 6
l6 24
23.0
24.4
22.6
26.0
24.00
42.6
9.2186
9.2479
13 3225
l6 30
13.0
13-1
II.7
11.6
12-35
38.7
8.6604
8.6826
0.6523
+ 1.63
6.46
13 3233
l6 32
13.8
15-4
15.0
14.4
14.65
39-o
8.8059
8.8286
0.5063
+ 1.27
6.10
10 3092
16 34
31*1
30.2
32-5
31.6
3i-35
42.1
9-4325
9.4608
0.1259
— 0.31
4-52
18 3266
l6 36
20.6
19.4
19.O
20.4
19.85
33-9
9.0618
9-0773
0.2576
+ 0.64
5-47
14 3179
l6 38
24.1
24.0
23.I
22.7
23.48
38.3
9.2007
9.2223
0.1126
4- 0.28
5-i 1
12 3142
l6 40
24.1
24.4
24.6
24-3
24-35
39-7
9-2305
9.2544
0.0805
+ 0.20
5-03
7 3023
l6 42
31-4
32.3
27.4
3i-3
30.60
46.4
9-4135
9-45I5
11 315 6
16 45
20.9
22.1
21.5
24-5
22.25
41.8
9-1565
9.1842
Mittel aus den Vergleicbsternbeobacbtungen: 9.3296; 9.3572; 9.3179. Zur Reduction benutzt: 9.3349.
Zone 595. 1892 Juni 16.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 36 und Nr. 38. Luft: 1
—2.
9°3424
15 k 2 5 in
3380
3080
33-4
3085
31872
49°7
9.4416
9.4889
10 3573
15 27
22.4
22.0
22.4
21.1
21.98
55-5
9.1464
9-2153
19 3435
15 30
27-5
25-5
28.8
24.2
26.50
42.1
.9.2991
9-3274
0.0193
— 0.05
6-33
18 3464
15 3 i
19.7
17.4
20.4
18.4
18.98
42.2
9.0244
9.0529
0.2552
+ O.64
7.02
19 34 i 6
15 33
10.0
7.6
10.5
8.0
9.02
4i-5
8.3906
8.4177
0.8904
+ 2.2 3
8.61
19 3401
15 35
13.0
11-5
13.0
12.4
12.48
40.8
8.6693
8.6951
0.6130
+ 1-53
7.91
17 3312
15 37
16.0
15-5
17.4
15-5
16.10
42.2
8.8859
8.9144
0.3937
-f- 0.98
7-36
15 3246
15 39
23.6
20.6
24.4
22.0
22.65
43-8
9.1712
9.2031
0.1050
+ 0.26
6.64
9 3424
15 4 i
29-5
29.6
32-4
29.0
30.12
48.1
9.4011
9-4437
10 3573
15 43
21.0
18.5
23.0
18.5
20.25
53-5
9.0785
9.1390
11 3251
i5 45
I9.6
16.6
19.8
17.0
18.25
47.2
8.9915
9.0316
0.2765
+ 0.69
7.07
14 3329
i5 47
24.6
24-5
26.8
23.0
24.72
44.0
9.2428
9-2751
0.0330
+ 0.08
6.46
14 3321
i5 49
25-5
22.6
26.6
22.5
24.30
43-8
9.2288
9.2607
0.0474
4-0.12
6.50
13 3444
15 50
19-5
18.0
18.6
16.7
18.20
44.2
8.9892
9.0220
0.2861
4- 0.72
7.10
13 3421
15 53
27.O
25-5
27.4
23-4
25.82
43-9
9.2780
9-3IOI
0.0020
— 0.01
6-37
13 3423
15 55
I3.6
11.2
12-5
13-5
12.70
43-9
8.6842
8.7163
0.5918
4- 1.48
7.86
9 3424
15 57
29.O
29.4
36.5
26.0
30.22
46.7
9-4037
9-4425
10 3573
15 59
20.6
20.6
21.0
17.6
19-95
5i-5
9.0660
1 9-ii9i
Mittel aus den Vergleichsternbeobachtungen: 9.3521; 9.2914; 9.2808.
Zur Reduction benutzt: 9.3081
